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Table of contentsALFA Pulsar Surveys Jim Cordes, Cornell University GALFA Workshop, Arecibo 20 March 2003 Boundary Conditions etc. Why more pulsars? Targeted Classes of Pulsars ALFA Pulsar Surveys Dmax vs. Flux Density Threshold Slide 7 Pulse broadening from multipath Implications: Comparison of AO, GBT & Parkes (Smin1 held fixed) Comparison of AO, GBT & Parkes Smin1 (AO) << Smin1 (Parkes) Nominal Parameters of Galactic Plane Survey PowerPoint Presentation Spectrometer Requirements II. Intermediate Latitude Survey Slide 16 Data Management What Next? Issues for Optimizing Surveys Pulsar Consortium Working Groups Slide 21 Preliminary Protocols |
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